4.7 Article

Barrow entropic dark energy: A member of generalized holographic dark energy family

Journal

PHYSICS LETTERS B
Volume 825, Issue -, Pages -

Publisher

ELSEVIER
DOI: 10.1016/j.physletb.2021.136844

Keywords

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Funding

  1. JSPS [18K03615]
  2. MINECO (Spain) [PID2019-104397GB-I00]

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In this study, the holographic cut-off in the formalism of generalized holographic dark energy (HDE) is generalized to depend on the particle horizon, future horizon, and scale factor of the universe. It is shown that the Barrow entropic dark energy (DE) model is equivalent to the generalized HDE, where the holographic cut-off is determined by the first-order derivative of the particle horizon or future horizon. The equivalence is extended to consider the variation of the Barrow entropy exponent with the cosmological expansion.
The holographic cut-off, in the formalism of generalized holographic dark energy (HDE), is generalized to depend on L-IR = L-IR(L-p, <(L)over dot>(p), <(L)double over dot>(p), center dot center dot center dot, L-f, <(L)over dot>(f), center dot center dot center dot, a), where L-p and L-f are the particle horizon and future horizon respectively, and a is the scale factor of the universe. Based on such formalism, we showed that the Barrow entropic dark energy (DE) model is equivalent to the generalized HDE where the respective holographic cut-off is determined by two ways - (1) in terms of particle horizon and its derivative and (2) in terms of future horizon and its derivative. Interestingly, such cut-off turns out to depend up-to first order derivative of L-p or L-f respectively. Such equivalence between the Barrow entropic dark energy and the generalized HDE is extended to the scenario where the exponent of the Barrow entropy allows to vary with the cosmological expansion of the universe. In both the cases (whether the Barrow exponent is a constant or varies with the cosmological evolution), we determine effective equation of state (EoS) parameter from the generalized holographic point of view, which, by comparing with the Barrow DE EoS parameter, further ensures the equivalence between the Barrow entropic dark energy and the generalized HDE. (C) 2021 The Author(s). Published by Elsevier B.V.

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